The primary physics goal of the RHIC project is to collide heavy nuclei with sufficient energy to produce a transition from hot, dense, hadronic matter to a color de-confined, chirally symmetric plasma of quarks and gluons (QGP). STAR will focus mainly on the investigation of soft processes resulting in hadron production at central rapidities and transverse momenta below 2 GeV/c but, in addition, will study hard QCD processes such as the production of jets, mini-jets and hard photons. STAR will also investigate nucleon structure functions and effects of quark and gluon shadowing through proton-proton and proton-nucleus interactions. The intent of the experimental program is to measure many observables, some of which are obtained on an event-by-event basis, and study their dependence on the size of the colliding system, the collision impact parameter and total energy.
The time evolution of nucleus-nucleus collisions is thought to involve
an initial parton scattering, pre-equilibrium stage, an intermediate
thermalization stage in which the QGP might be formed, and a final expansion
and hadronization stage. Observables can be associated with each stage
which convey different information about the collision dynamics. For example,
hard parton scatterings in the initial pre-equilibrium stage result in high
particles, jets, high energy 
s, and charmed mesons.
Conditions during the intermediate thermalization stage ( i.e., hot
hadronic gas or QGP) affect the production of mini-jets, strangeness,
anti-baryons, isospin anomalies and energy/entropy fluctuations.
Multi-strange baryon and 
meson production are strongly dependent on
strangeness density during this stage and are therefore sensitive
indicators of possible chiral symmetry restoration in the QGP. Global
properties such as size and temperature during the final hadronization
stage can be determined by the 
spectra and by 
and KK
HBT interferometry.
The baseline configuration of the STAR detector consists of a large
room temperature solenoidal magnet, a time projection chamber (TPC)
for charged particle tracking, and trigger counters (vertex position
detectors, central trigger barrel). Charged particle momenta will be
measured with the TPC at mid-rapidity (
) with full
azimuthal coverage and a transverse momentum, 
, threshold
of about 150 MeV/c. Particle identification through measurement of
ionization density (dE/dx) will be accomplished for particles emitted
with 
and 
MeV/c.
With the TPC alone, STAR is limited to the study of hadron production
with 
above 150 MeV/c and has a modest efficiency and
accuracy for the study of short lived particles decaying before they
reach the inner layer of the TPC. Multi-strange baryons and
anti-baryons cannot be studied with the STAR baseline detector.
The purpose of the STAR Silicon Vertex Tracker (SVT) upgrade is to provide
unique capabilities
for the measurement of several of the preceding list of observables as well
as to enhance the overall performance of STAR. Unique capabilities of
the SVT include the detection of multi-strange baryons
(
and 
) and measurement of low 
(40 
200 MeV/c) spectra.
Measurements of rare particles such as the D mesons
and strange composite objects, which are impossible to
observe with the TPC alone, might become accessible with the SVT.
The SVT will provide substantial improvement in the momentum resolution
for high 
particles, in the reconstruction efficiency
for short lived neutral particles such as 
, 
, 
, and
, and in two-track resolution for HBT studies
owing to the excellent position resolution achievable with Si drift
chamber technology.
The SVT will also enhance track reconstruction and particle
identification for soft charged particles such as 
, 
, p, 
, d and 
,
will enable better determination of the primary vertex, and will
help distinguish particles resulting from secondary decays.
It is unlikely that conclusive evidence of QGP formation at RHIC can be based on a single observable or signature; instead we will require the simultaneous observation of many signatures. It is expected that only a consistent analysis of many signals coming from all stages of the collision may lead to an unambiguous identification of the phase transition. STAR complemented with the SVT represents a powerful instrument for studying this possible transition to a new state of matter.
A detailed description of the integrated STAR system (baseline detector plus upgrades) can be found in the original STAR conceptual design report (CDR) [[1]].
In this document, we outline a proposal
for the construction of an SVT for STAR which uniquely addresses
low-
and flavor physics otherwise unsatisfactorily
covered by other RHIC detectors.